Whitworth, Anthony ORCID: https://orcid.org/0000-0002-1178-5486, Priestley, Felix and Geen, S T 2022. Ionizing feedback from an O star formed in a shock-compressed layer. Monthly Notices of the Royal Astronomical Society 517 (4) , pp. 4940-4949. 10.1093/mnras/stac2955 |
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Abstract
We develop a simple analytical model for what happens when an O star (or compact cluster of OB stars) forms in a shock-compressed layer and carves out an approximately circular hole in the layer, at the waist of a bipolar H II region (H IIR). The model is characterized by three parameters: the half-thickness of the undisturbed layer, ZLAYER, the mean number density of hydrogen molecules in the undisturbed layer, nLAYER, and the (collective) ionizing output of the star(s), N˙LyC. The radius of the circular hole is given by WIF(t)∼3.8pc[ZLAYER/0.1pc]−1/6[nLAYER/104cm−3]−1/3[N˙LyC/1049s−1]1/6[t/Myr]2/3. Similar power-law expressions are obtained for the rate at which ionized gas is fed into the bipolar lobes, the rate at which molecular gas is swept up into a dense ring by the shock front that precedes the ionization front, and the density in this dense ring. We suggest that our model might be a useful zeroth-order representation of many observed H IIRs. From viewing directions close to the mid-plane of the layer, the H IIR will appear bipolar. From viewing directions approximately normal to the layer, it will appear to be a limb-brightened shell but too faint through the centre to be a spherically symmetric bubble. From intermediate viewing angles, more complicated morphologies can be expected.
Item Type: | Article |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Publisher: | Royal Astronomical Society |
ISSN: | 0035-8711 |
Date of First Compliant Deposit: | 4 January 2023 |
Date of Acceptance: | 11 October 2022 |
Last Modified: | 09 May 2023 00:11 |
URI: | https://orca.cardiff.ac.uk/id/eprint/155295 |
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